The most mysterious star in the universe Tabetha Boyajian

Extraordinary claims
require extraordinary evidence,

and it is my job,
my responsibility, as an astronomer

to remind people that alien hypotheses
should always be a last resort.

Now, I want to tell you
a story about that.

It involves data from a NASA mission,

ordinary people and one of the most
extraordinary stars in our galaxy.

It began in 2009 with the launch
of NASA’s Kepler mission.

Kepler’s main scientific objective

was to find planets
outside of our solar system.

It did this by staring
at a single field in the sky,

this one, with all the tiny boxes.

And in this one field,

it monitored the brightness
of over 150,000 stars

continuously for four years,

taking a data point every 30 minutes.

It was looking for what
astronomers call a transit.

This is when the planet’s orbit
is aligned in our line of sight,

just so that the planet
crosses in front of a star.

And when this happens,
it blocks out a tiny bit of starlight,

which you can see as a dip in this curve.

And so the team at NASA
had developed very sophisticated computers

to search for transits
in all the Kepler data.

At the same time
of the first data release,

astronomers at Yale
were wondering an interesting thing:

What if computers missed something?

And so we launched the citizen
science project called Planet Hunters

to have people look at the same data.

The human brain has an amazing ability
for pattern recognition,

sometimes even better than a computer.

However, there was a lot
of skepticism around this.

My colleague, Debra Fischer,
founder of the Planet Hunters project,

said that people at the time were saying,

“You’re crazy. There’s no way
that a computer will miss a signal.”

And so it was on, the classic
human versus machine gamble.

And if we found one planet,
we would be thrilled.

When I joined the team four years ago,

we had already found a couple.

And today, with the help
of over 300,000 science enthusiasts,

we have found dozens,

and we’ve also found
one of the most mysterious stars

in our galaxy.

So to understand this,

let me show you what a normal transit
in Kepler data looks like.

On this graph on the left-hand side
you have the amount of light,

and on the bottom is time.

The white line
is light just from the star,

what astronomers call a light curve.

Now, when a planet transits a star,
it blocks out a little bit of this light,

and the depth of this transit
reflects the size of the object itself.

And so, for example, let’s take Jupiter.

Planets don’t get
much bigger than Jupiter.

Jupiter will make a one percent drop
in a star’s brightness.

Earth, on the other hand,
is 11 times smaller than Jupiter,

and the signal
is barely visible in the data.

So back to our mystery.

A few years ago, Planet Hunters were
sifting through data looking for transits,

and they spotted a mysterious signal
coming from the star KIC 8462852.

The observations in May of 2009
were the first they spotted,

and they started talking about this
in the discussion forums.

They said and object like Jupiter

would make a drop like this
in the star’s light,

but they were also saying it was giant.

You see, transits normally
only last for a few hours,

and this one lasted for almost a week.

They were also saying
that it looks asymmetric,

meaning that instead of the clean,
U-shaped dip that we saw with Jupiter,

it had this strange slope
that you can see on the left side.

This seemed to indicate

that whatever was getting in the way
and blocking the starlight

was not circular like a planet.

There are few more dips that happened,

but for a couple of years,
it was pretty quiet.

And then in March of 2011, we see this.

The star’s light drops
by a whole 15 percent,

and this is huge compared to a planet,

which would only make a one percent drop.

We described this feature
as both smooth and clean.

It also is asymmetric,

having a gradual dimming
that lasts almost a week,

and then it snaps right back up to normal
in just a matter of days.

And again, after this, not much happens

until February of 2013.

Things start to get really crazy.

There is a huge complex of dips
in the light curve that appear,

and they last for like a hundred days,

all the way up
into the Kepler mission’s end.

These dips have variable shapes.

Some are very sharp, and some are broad,

and they also have variable durations.

Some last just for a day or two,
and some for more than a week.

And there’s also up and down trends
within some of these dips,

almost like several independent events
were superimposed on top of each other.

And at this time, this star drops
in its brightness over 20 percent.

This means that whatever
is blocking its light

has an area of over 1,000 times
the area of our planet Earth.

This is truly remarkable.

And so the citizen scientists,
when they saw this,

they notified the science team
that they found something weird enough

that it might be worth following up.

And so when the science team looked at it,

we’re like, “Yeah, there’s probably
just something wrong with the data.”

But we looked really, really, really hard,

and the data were good.

And so what was happening
had to be astrophysical,

meaning that something in space
was getting in the way

and blocking starlight.

And so at this point,

we set out to learn
everything we could about the star

to see if we could find any clues
to what was going on.

And the citizen scientists
who helped us in this discovery,

they joined along for the ride

watching science in action firsthand.

First, somebody said, you know,
what if this star was very young

and it still had the cloud of material
it was born from surrounding it.

And then somebody else said,

well, what if the star
had already formed planets,

and two of these planets had collided,

similar to the Earth-Moon forming event.

Well, both of these theories
could explain part of the data,

but the difficulties were that the star
showed no signs of being young,

and there was no glow
from any of the material

that was heated up by the star’s light,

and you would expect this
if the star was young

or if there was a collision
and a lot of dust was produced.

And so somebody else said,

well, how about a huge swarm of comets

that are passing by this star
in a very elliptical orbit?

Well, it ends up that this is actually
consistent with our observations.

But I agree, it does feel
a little contrived.

You see, it would take hundreds of comets

to reproduce what we’re observing.

And these are only the comets

that happen to pass
between us and the star.

And so in reality, we’re talking
thousands to tens of thousands of comets.

But of all the bad ideas we had,

this one was the best.

And so we went ahead
and published our findings.

Now, let me tell you, this was one
of the hardest papers I ever wrote.

Scientists are meant to publish results,

and this situation was far from that.

And so we decided
to give it a catchy title,

and we called it: “Where’s The Flux?”

I will let you work out the acronym.

(Laughter)

So this isn’t the end of the story.

Around the same time
I was writing this paper,

I met with a colleague
of mine, Jason Wright,

and he was also writing a paper
on Kepler data.

And he was saying that with Kepler’s
extreme precision,

it could actually detect
alien megastructures around stars,

but it didn’t.

And then I showed him this weird data
that our citizen scientists had found,

and he said to me,

“Aw crap, Tabby.

Now I have to rewrite my paper.”

So yes, the natural
explanations were weak,

and we were curious now.

So we had to find a way
to rule out aliens.

So together, we convinced
a colleague of ours

who works on SETI, the Search
for Extraterrestrial Intelligence,

that this would be
an extraordinary target to pursue.

We wrote a proposal to observe the star

with the world’s largest radio telescope
at the Green Bank Observatory.

A couple months later,

news of this proposal
got leaked to the press

and now there are thousands of articles,

over 10,000 articles, on this star alone.

And if you search Google Images,

this is what you’ll find.

Now, you may be wondering,
OK, Tabby, well,

how do aliens actually explain
this light curve?

OK, well, imagine a civilization
that’s much more advanced than our own.

In this hypothetical circumstance,

this civilization would have exhausted
the energy supply of their home planet,

so where could they get more energy?

Well, they have a host star
just like we have a sun,

and so if they were able
to capture more energy from this star,

then that would solve their energy needs.

So they would go
and build huge structures.

These giant megastructures,

like ginormous solar panels,
are called Dyson spheres.

This image above

are lots of artists' impressions
of Dyson spheres.

It’s really hard to provide perspective
on the vastness of these things,

but you can think of it this way.

The Earth-Moon distance
is a quarter of a million miles.

The simplest element
on one of these structures

is 100 times that size.

They’re enormous.

And now imagine one of these structures
in motion around a star.

You can see how it would produce
anomalies in the data

such as uneven, unnatural looking dips.

But it remains that even
alien megastructures

cannot defy the laws of physics.

You see, anything that uses
a lot of energy

is going to produce heat,

and we don’t observe this.

But it could be something as simple

as they’re just reradiating it away
in another direction,

just not at Earth.

Another idea that’s one
of my personal favorites

is that we had just witnessed
an interplanetary space battle

and the catastrophic
destruction of a planet.

Now, I admit that this
would produce a lot of dust

that we don’t observe.

But if we’re already invoking aliens
in this explanation,

then who is to say they didn’t
efficiently clean up all this mess

for recycling purposes?

(Laughter)

You can see how this quickly
captures your imagination.

Well, there you have it.

We’re in a situation that could unfold

to be a natural phenomenon
we don’t understand

or an alien technology
we don’t understand.

Personally, as a scientist,
my money is on the natural explanation.

But don’t get me wrong, I do think
it would be awesome to find aliens.

Either way, there is something new
and really interesting to discover.

So what happens next?

We need to continue to observe this star

to learn more about what’s happening.

But professional astronomers, like me,

we have limited resources
for this kind of thing,

and Kepler is on to a different mission.

And I’m happy to say that once again,

citizen scientists have come in
and saved the day.

You see, this time,

amateur astronomers
with their backyard telescopes

stepped up immediately
and started observing this star nightly

at their own facilities,

and I am so excited to see what they find.

What’s amazing to me is that this star
would have never been found by computers

because we just weren’t looking
for something like this.

And what’s more exciting

is that there’s more data to come.

There are new missions that are coming up

that are observing millions more stars

all over the sky.

And just think: What will it mean
when we find another star like this?

And what will it mean
if we don’t find another star like this?

Thank you.

(Applause)

非凡的主张
需要非凡的证据

,作为一名天文学家,我的工作和责任

是提醒人们外星人的假设
应该永远是最后的手段。

现在,我想给你讲
一个关于它的故事。

它涉及来自 NASA 任务、

普通人和
我们银河系中最非凡的恒星之一的数据。

它始于 2009 年
NASA 开普勒任务的启动。

开普勒的主要科学目标

是寻找
太阳系外的行星。

它通过
盯着天空中的一个领域来做到这一点,

这个领域,所有的小盒子。

而在这一领域,

它连续四年监测
超过15万颗恒星的亮度,

每30分钟采集一个数据点。

它正在寻找
天文学家所说的凌日。

这是当行星的
轨道与我们的视线对齐时

,行星正好
穿过一颗恒星的前面。

当这种情况发生时,
它会挡住一点点星光

,你可以看到它是这条曲线的一个下降点。

因此,美国宇航局的团队
开发了非常复杂的计算机

来搜索
所有开普勒数据中的过境。


第一次数据发布的同时,

耶鲁大学的天文学家
想知道一件有趣的事情:

如果计算机遗漏了什么怎么办?

因此,我们启动了
名为 Planet Hunters 的公民科学项目

,让人们查看相同的数据。

人脑具有惊人
的模式识别能力,

有时甚至比计算机还要好。

然而,对此有
很多怀疑。

我的同事,
行星猎人项目的创始人黛布拉·菲舍尔

说,当时人们在说,

“你疯了
。计算机不可能错过任何信号。”

就这样,经典的
人与机器博弈开始了。

如果我们找到一颗行星,
我们会很激动。

四年前我加入团队时,

我们已经找到了一对。

而今天,在
超过 300,000 名科学爱好者的帮助下,

我们发现了数十颗,

而且我们还发现
了银河系中最神秘的恒星

之一。

因此,为了理解这一点,

让我向您
展示开普勒数据中的正常传输是什么样的。

在这张图表的
左边是光量

,底部是时间。

白线
是来自恒星

的光,天文学家称之为光曲线。

现在,当一颗行星凌日一颗恒星时,
它会阻挡一点这种光,

而这种凌日的深度
反映了物体本身的大小。

因此,例如,让我们以木星为例。

行星不会
比木星大多少。

木星会使
恒星的亮度下降百分之一。

另一方面,地球
比木星小 11 倍,

数据中几乎看不到信号。

所以回到我们的谜团。

几年前,行星猎人在
筛选数据以寻找凌日

,他们发现了
来自恒星 KIC 8462852

的神秘信号。2009 年 5 月的观测
是他们发现的第一个

,他们开始
在论坛上讨论这个问题 .

他们说像木星

这样的天体会
在恒星的光线下像这样落下,

但他们也说它是巨大的。

你看,过境通常
只持续几个小时,

而这次持续了将近一周。

他们
还说它看起来不对称,

这意味着它不是
我们在木星上看到的干净的 U 形倾斜,

而是有
一个你可以在左侧看到的奇怪斜坡。

这似乎表明

,任何
阻碍星光的东西

都不像行星那样是圆形的。

发生了几次下跌,

但几年来,
它非常安静。

然后在 2011 年 3 月,我们看到了这一点。

这颗恒星的光
下降了整整 15%,

与一颗只会下降 1% 的行星相比,这是巨大的

我们将此功能描述
为既流畅又干净。

它也是不对称的

,逐渐
变暗持续近一周,

然后在短短几天内立即恢复正常

再一次,在此之后,

直到 2013 年 2 月才发生太多事情。

事情开始变得非常疯狂。

光变曲线中出现了一个巨大的下降复合体

,它们持续了大约一百天,

一直
到开普勒任务的结束。

这些倾角具有可变的形状。

有些非常尖锐,有些很广泛,

而且它们的持续时间也不同。

有些只持续一两天
,有些持续一周以上。 在这些下跌中

也有上升和下降趋势

几乎就像几个独立的
事件叠加在一起一样。

而此时,这颗恒星
的亮度下降了 20% 以上。

这意味着
任何阻挡其光线的

物体的面积都是地球面积的 1000 多倍。

这真是了不起。

所以公民科学家,
当他们看到这一点时,

他们通知科学
团队他们发现了一些非常奇怪

的东西,可能值得跟进。

因此,当科学团队查看它时,

我们会说,“是的,
可能只是数据有问题。”

但是我们看起来非常非常非常努力,

而且数据很好。

所以发生的事情
必须是天体物理学,

这意味着太空中的某些东西

挡住了星光。

所以在这一点上,

我们开始尽可能地
了解这颗恒星的一切

,看看我们是否能找到任何线索
来了解正在发生的事情。


在这一发现中帮助我们的公民科学家

们也加入了这一

行列,亲眼目睹了科学的实际应用。

首先,有人说,你知道,
如果这颗恒星非常年轻,

而且它周围还有一团物质云,
它是从它周围诞生的。

然后有人说,

好吧,如果这颗恒星
已经形成了行星,

其中两个行星发生了碰撞,

类似于地球-月球形成事件。

嗯,这两种理论
都可以解释部分数据,

但困难在于这颗恒星
没有年轻的迹象,

而且

任何被恒星光加热的物质都没有发光

,你会期待
如果这颗恒星很年轻,

或者发生碰撞
并产生大量尘埃,就会出现这种情况。

所以有人说,

好吧,一大群彗星

在一个非常椭圆的轨道上经过这颗恒星怎么样?

好吧,最终这实际上
与我们的观察结果一致。

但我同意,它确实感觉
有点做作。

你看,需要数百颗彗星

来重现我们正在观察的东西。

而这些

只是碰巧
在我们和恒星之间经过的彗星。

所以实际上,我们说的
是成千上万的彗星。

但在我们所有的坏主意中,

这个是最好的。

所以我们
继续发表了我们的发现。

现在,让我告诉你,这是
我写过的最难的论文之一。

科学家的本意是要公布结果,

而这种情况远非如此。

所以我们决定
给它起一个醒目的标题

,我们称之为:“通量在哪里?”

我会让你计算出首字母缩写词。

(笑声)

所以这不是故事的结局。

大约在
我写这篇论文的同时,

我遇到了我的一位同事
Jason Wright

,他也在写一篇
关于开普勒数据的论文。

他是说,以开普勒的
极高精确度,

它实际上可以探测到
恒星周围的外星巨型结构,

但它没有。

然后我向他展示了
我们的公民科学家发现的这些奇怪的数据

,他对我说,

“废话,Tabby。

现在我必须重写我的论文。”

所以是的,自然
解释很弱

,我们现在很好奇。

所以我们必须想
办法排除外星人。

因此,我们一起说服
了我们的

一位从事 SETI(
寻找外星智能)工作的同事,

相信这将是
一个非常值得追求的目标。

我们写了一份提案,在绿岸天文台

用世界上最大的射电望远镜观察这颗恒星

几个月后,

该提议的消息
被泄露给了媒体

,现在

仅在这颗星上就有数千篇文章,超过 10,000 篇文章。

如果你搜索谷歌图片

,你会找到这个。

现在,您可能想知道,
好吧,Tabby,好吧,

外星人实际上是如何解释
这种光变曲线的?

好吧,好吧,想象一个
比我们自己先进得多的文明。

在这种假设的情况下,

这个文明本来应该已经耗尽
了他们家乡星球的能源供应,

那么他们还能从哪里获得更多的能源呢?

嗯,他们有一颗主星
,就像我们有太阳一样

,所以如果他们能够
从这颗恒星中捕获更多的能量,

那么这将解决他们的能量需求。

所以他们会
去建造巨大的结构。

这些巨大的巨型结构,

如巨大的太阳能电池板,
被称为戴森球。

上图

是很多艺术家
对戴森球的印象。

很难就
这些事物的浩瀚提供视角,

但你可以这样想。

地月距离
是一百万英里的四分之一。

其中一个结构上最简单的元素

是该大小的 100 倍。

他们是巨大的。

现在想象其中一个
围绕恒星运动的结构。

您可以看到它如何
在数据中产生异常,

例如不均匀、看起来不自然的下降。

但即使是
外星巨型结构

也不能违背物理定律。

你看,任何
消耗大量能量

的东西都会产生热量,

而我们没有观察到这一点。

但这可能很简单,

因为他们只是将其重新辐射
到另一个方向,

而不是在地球上。

我个人最喜欢的另一个想法

是,我们刚刚目睹
了一场星际太空战斗


一颗行星的灾难性破坏。

现在,我承认这
会产生很多

我们没有观察到的灰尘。

但是,如果我们已经
在这个解释中引用了外星人,

那么谁能说他们没有
有效地清理所有这些烂摊子

以进行回收利用呢?

(笑声)

你可以看到这如何迅速地
激发了你的想象力。

好吧,你有它。

我们所处的情况可能

会演变成一种我们不了解的自然现象

或一种我们不了解的外星技术

就个人而言,作为一名科学家,
我的钱花在了自然解释上。

但不要误会我的意思,我确实
认为找到外星人会很棒。

无论哪种方式,都会有一些新的
和非常有趣的发现。

那么接下来会发生什么?

我们需要继续观察这颗恒星,

以了解更多关于正在发生的事情。

但是像我这样的专业天文学家,

我们在
这类事情上的资源有限,

而开普勒正在执行不同的任务。

我很高兴再次重申,

公民科学家的
到来挽救了局面。

你看,这一次,

业余天文学家
带着他们的后院望远镜

立即站出来
,开始

在他们自己的设施中每晚观察这颗恒星

,我很高兴看到他们发现了什么。

令我惊讶的是,这颗恒星
永远不会被计算机发现,

因为我们只是没有在寻找
这样的东西。

更令人兴奋

的是还有更多的数据。

即将出现的新任务将在天空

中观测数百万颗恒星

想一想:
当我们找到另一颗这样的恒星时,这意味着什么?

如果我们找不到另一颗这样的恒星,这意味着什么?

谢谢你。

(掌声)